معرفی شرکت ها


firstgalaxydata-0.2.1


Card image cap
تبلیغات ما

مشتریان به طور فزاینده ای آنلاین هستند. تبلیغات می تواند به آنها کمک کند تا کسب و کار شما را پیدا کنند.

مشاهده بیشتر
Card image cap
تبلیغات ما

مشتریان به طور فزاینده ای آنلاین هستند. تبلیغات می تواند به آنها کمک کند تا کسب و کار شما را پیدا کنند.

مشاهده بیشتر
Card image cap
تبلیغات ما

مشتریان به طور فزاینده ای آنلاین هستند. تبلیغات می تواند به آنها کمک کند تا کسب و کار شما را پیدا کنند.

مشاهده بیشتر
Card image cap
تبلیغات ما

مشتریان به طور فزاینده ای آنلاین هستند. تبلیغات می تواند به آنها کمک کند تا کسب و کار شما را پیدا کنند.

مشاهده بیشتر
Card image cap
تبلیغات ما

مشتریان به طور فزاینده ای آنلاین هستند. تبلیغات می تواند به آنها کمک کند تا کسب و کار شما را پیدا کنند.

مشاهده بیشتر

توضیحات

-
ویژگی مقدار
سیستم عامل -
نام فایل firstgalaxydata-0.2.1
نام firstgalaxydata
نسخه کتابخانه 0.2.1
نگهدارنده []
ایمیل نگهدارنده []
نویسنده Florian Griese
ایمیل نویسنده -
آدرس صفحه اصلی -
آدرس اینترنتی https://pypi.org/project/firstgalaxydata/
مجوز -
# Radio Galaxy Dataset [![DOI](https://zenodo.org/badge/DOI/10.5281/zenodo.7120632.svg)](https://doi.org/10.5281/zenodo.7120632) [![License](https://img.shields.io/github/license/floriangriese/RadioGalaxyDataset?color=green&style=flat)](https://github.com/floriangriese/RadioGalaxyDataset/blob/main/LICENSE) This Radio Galaxy Dataset is a collection and combination of several catalogues using the FIRST radio galaxy survey [[1]](https://ui.adsabs.harvard.edu/abs/1995ApJ...450..559B/abstract). To the images from the FIRST radio galaxy survey the following license applies: "Provenance: The FIRST project team: R.J. Becker, D.H. Helfand, R.L. White M.D. Gregg. S.A. Laurent-Muehleisen. Copyright: 1994, University of California. Permission is granted for publication and reproduction of this material for scholarly, educational, and private non-commercial use. Inquiries for potential commercial uses should be addressed to: Robert Becker, Physics Dept, University of California, Davis, CA 95616: Further, the following catalogues are included in this dataset: * MiraBest [[2]](https://academic.oup.com/mnras/article/466/4/4346/2843096), [Source](https://zenodo.org/record/4288837#.YFSBEdwxlaT) * Gendre [[3-4]](https://academic.oup.com/mnras/article/404/4/1719/1081038?login=true), Supplementary Data: mnras0404-1719-SD1.pdf, data tables CoNFIG-1 to CoNFIG-4 * Capetti 2017a [[5]](https://www.aanda.org/articles/aa/full_html/2017/02/aa29287-16/aa29287-16.html), [Table](https://www.aanda.org/articles/aa/full_html/2017/02/aa29287-16/T1.html) * Capetti 2017b [[6]](https://www.aanda.org/articles/aa/full_html/2017/05/aa30247-16/aa30247-16.html), [Table](http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/601/A81) * Baldi 2018 [[7]](https://www.aanda.org/articles/aa/full_html/2018/01/aa31333-17/aa31333-17.html), [Table](https://www.aanda.org/articles/aa/full_html/2018/01/aa31333-17/T1.html) * Proctor [[8]](https://ui.adsabs.harvard.edu/abs/2011ApJS..194...31P/abstract), [Table](https://iopscience.iop.org/article/10.1088/0067-0049/194/2/31#apjs390184t1), data from Table 1 with label “WAT” and “NAT” Examples for the class definitions of FRI, FRII, Compact and Bent are shown below, ![image](img/Classification_Scheme.png) with the labels | classes | Label | | ----------- | ----------- | | FRI | 0 | | FRII | 1 | | Compact| 2 | | Bent | 3 | The dataset has the following total number of samples per class. | classes/split | FRI | FRII | Compact | Bent | Total | | ----------- | ----------- |----------- |----------- |----------- |-----------| | total | 495 |924 |391 |348 |2158 | We provide two splitting options for the dataset. The first splitting option (galaxy_data_h5.zip) provides three splittings in train, valid and test with the following number of sample per class. | classes/split | FRI | FRII | Compact | Bent | Total | | ----------- | ----------- |----------- |----------- |----------- |-----------| | train | 395 |824 |291 |248 |1758 | | valid | 50 | 50 | 50 | 50 |200 | | test | 50 | 50 | 50 | 50 |200 | | total | 495 |924 |391 |348 |2158 | The second splitting option (galaxy_data_crossvalid_0_h5.zip to galaxy_data_crossvalid_4_h5.zip and galaxy_data_crossvalid_test_h5.zip) provides a 5-fold cross validation dataset with a larger test set. | classes/split | FRI | FRII | Compact | Bent | Total | | ----------- | ----------- |----------- |----------- |----------- |-----------| | 5-fold cross train | 316 | 659 | 232 | 198 |1405 | | 5-fold cross valid | 79 | 165 | 59 | 50 |353 | | test | 100 | 100 | 100 | 100 |400 | | total | 495 |924 |391 |348 |2158 | # Installation usage with pytorch If you want to use the dataset via the dataset class `FIRSTGalaxyData` with pytorch, install the necessary packages with `pip3 install -r requirements.txt` first, otherwise you can use the dataset * directly with *.png files on disk or * load the dataset directly from the HDF5 file. Both options are descibed further below. # Usage with pytorch ``` from firstgalaxydata import FIRSTGalaxyData import torchvision.transforms as transforms ``` ``` transformRGB = transforms.Compose( [transforms.ToTensor(), transforms.Normalize(mean=[0.5, 0.5, 0.5], std=[0.5, 0.5, 0.5])]) ``` ``` data = FIRSTGalaxyData(root="./", selected_split="train", input_data_list=["galaxy_data_h5.h5"], is_PIL=True, is_RGB=True, transform=transformRGB) ``` ```print(data)``` This will print out the following output: ```Dataset FIRSTGalaxyData Selected classes: dict_values(['FRI', 'FRII', 'Compact', 'Bent']) Number of datapoints in total: 1758 Number of datapoint in class FRI: 395 Number of datapoint in class FRII: 824 Number of datapoint in class Compact: 291 Number of datapoint in class Bent: 248 Split: train Root Location: ./ Transforms (if any): Compose( ToTensor() Normalize(mean=[0.5, 0.5, 0.5], std=[0.5, 0.5, 0.5]) ) Target Transforms (if any): None ``` ## Options With `selected_split` the data split is selected. Choose either `"train"` or `"valid"` or `"test"`. With `selected_classes` only data containing the chosen classes is returned. e.g. `["FRI",FRII"]` returns only FRI and FRII images. With `selected_catalogues` the dataset uses only the selected catalogues. All possible catalogues are listed here: `selected_catalogues= ["Gendre", "MiraBest", "Capetti2017a", "Capetti2017b", "Baldi2018", "Proctor_Tab1"]` ```data = FIRSTGalaxyData(root="./", selected_split="train", input_data_list=["galaxy_data_h5.h5"], selected_catalogues=selected_catalogues, is_PIL=True, is_RGB=True, transform=transformRGB)``` # Basic usage with files on disk You will also find the dataset in the 'galaxy_data' folder by unzipping `galaxy_data.zip`. It contains the following folder sturcture with *.png images. The most import information will also be part of the file name separated by underscores: `RA_DEC_Label_Source.png` E.g. `14.084_-9.608_3_MiraBest.png` ``` galaxy_data │ └───all │ │ Bent | | *.png │ │ Compact | | *.png | | FRI | | *.png │ │ FRII | | *.png │ └───test │ │ Bent | | *.png │ │ Compact | | *.png | | FRI | | *.png │ │ FRII | | *.png │ └───train │ │ Bent | | *.png │ │ Compact | | *.png | | FRI | | *.png │ │ FRII | | *.png │ └───valid │ │ Bent | | *.png │ │ Compact | | *.png | | FRI | | *.png │ │ FRII | | *.png ``` # Basic usage with HDF5 file The dataset can also be accessed via the HDF5 file `galaxy_data_h5.h5`. Every data entry consists of a group named `data_$(i)` with `i=1...n` where `n` is the total number of data entries. Each group consists of the following data: * `Img`: two-dimensional uint8 array with (300,300) * Attributes of `Img`: * `RA` right ascension equatorial coordinate system (J2000): double * `DEC` declination equatorial coordinate system (J2000): double * `Source`: string, ["Gendre", "MiraBest", "Capetti2017a", "Capetti2017b", "Baldi2018", "Proctor_Tab1"] * `Filepath_literature`: string, relative path to the *.png file in the folder `galaxy_data` * `Label_literature`: double scalar, 0: ”FRI”, 1: ”FRII”, 2: ”Compact”, 3: ”Bent” * `Split_literature`: string, ["train","test","valid"] # References [1] R. H. Becker, R. L. White, D. J. Helfand, The FIRST Survey: Faint Images of the Radio Sky at Twenty Centimeters, The Astrophysical Journal 450 (1995) 559. [2] H. Miraghaei, P. N. Best, The nuclear properties and extended morphologies of powerful radio galaxies: the roles of host galaxy and environment, Monthly Notices of the Royal Astronomical Society (2017) stx007. [3] M. A. Gendre, P. N. Best, J. V. Wall, The combined nvss-first galaxies (config) sample - ii. comparison of space densities in the fanaroff-riley dichotomy, Monthly Notices of the Royal Astronomical Society (2010). [4] M. A. Gendre, J. V. Wall, The combined nvss-first galaxies (config) sample - i. sample definition, classification and evolution, Monthly Notices of the Royal Astronomical Society (2008). [5] A. Capetti, F. Massaro, R. D. Baldi, Fricat: A first catalog of fr i radio galaxies, Astronomy & Astrophysics 598 (2017) A49. [6] A. Capetti, F. Massaro, R. D. Baldi, Friicat: A first catalog of fr ii radio galaxies, Astronomy & Astrophysics 601 (2017) A81. [7] R. D. Baldi, A. Capetti, F. Massaro, Fr0cat: a first catalog of fr 0 radio galaxies, Astronomy & Astrophysics 609 (2017) A1. [8] D. D. Proctor, Morphological annotations for groups in the first database, The Astrophysical Journal Supplement Series 194 (2011) 31.


نیازمندی

مقدار نام
- numpy
- pillow
- torch
- torchvision
- astropy
- matplotlib
- h5py


زبان مورد نیاز

مقدار نام
>=3.6 Python


نحوه نصب


نصب پکیج whl firstgalaxydata-0.2.1:

    pip install firstgalaxydata-0.2.1.whl


نصب پکیج tar.gz firstgalaxydata-0.2.1:

    pip install firstgalaxydata-0.2.1.tar.gz